Abstract
This chapter aims at characterizing and modeling solar resource variability. It is shown that understanding solar energy variability requires a definition of the temporal and spatial context for which variability is assessed. This research describes a predictable, quantifiable variability-smoothing space–time continuum from a single point to thousands of kilometers and from seconds to days. Implications for solar penetration on the power grid and variability mitigation strategies are also discussed. Models for predicting intra-day or intra-hourly variability as a function of insolation conditions are also depicted.
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Notes
- 1.
This velocity is a priori defined as the vector in the direction of the two considered locations. However, as will be discussed below, empirical evidence shows that a mean, local—directionless—velocity, can be an adequate input for assessing regional station pair correlations.
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Acknowledgement
This chapter includes material originally developed for articles written in collaboration with Jan Kleissl of University of San Diego, California.
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Perez, R., Lauret, P., Perez, M., David, M., Hoff, T.E., Kivalov, S. (2018). Solar Resource Variability. In: Perez, R. (eds) Wind Field and Solar Radiation Characterization and Forecasting. Green Energy and Technology. Springer, Cham. https://doi.org/10.1007/978-3-319-76876-2_7
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